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FOr the beginning, adde to the minutes of Incidence the motion of the Sun agreeing to the time of Incidence, and the summe sub∣tract from the true motion of latitude at the time of the visible Sy∣nod, so have you the true motion of latitude at the beginning, by which find the true latitude, and by these according to the second rule of the 32 Chapter, may be had the visible latitude.
2 For the end, adde to the minutes of incidence the motion of the Sun agreeing to the time of repletion and the sum adde to the true motion of latitude at the time of the visible Conjunction; so have you the true moti∣on of latitude at the end; by which proceed as before, to find the visible Latitude.